characterization of arradiance samples and b33 float glass slade j. jokela
DESCRIPTION
SEY of Arradiance Samples No clear trend between scans Each scan was approximately 5 minutes long Approximately 200nA (electrons) continuousTRANSCRIPT
![Page 1: Characterization of Arradiance Samples and B33 Float Glass Slade J. Jokela](https://reader036.vdocuments.us/reader036/viewer/2022082510/5a4d1b2a7f8b9ab059998a6c/html5/thumbnails/1.jpg)
Characterization of Arradiance Samples and B33 Float Glass
Slade J. Jokela
![Page 2: Characterization of Arradiance Samples and B33 Float Glass Slade J. Jokela](https://reader036.vdocuments.us/reader036/viewer/2022082510/5a4d1b2a7f8b9ab059998a6c/html5/thumbnails/2.jpg)
XPS of Arradiance Samples
arr2-xps.1
O 1s
Al 2p
C 1s
F 1s
x 104
5
10
15
20
CPS
700 600 500 400 300 200 100 0Bi nding E nergy (eV)
F
O
CAl
Sample %O %Al %F %C
ARR1 51.02 32.35 2.15 14.48
ARR2 51.81 31.97 2.12 14.10
ARR3 53.51 31.61 2.40 12.48
•Samples are practically identical according to XPS
![Page 3: Characterization of Arradiance Samples and B33 Float Glass Slade J. Jokela](https://reader036.vdocuments.us/reader036/viewer/2022082510/5a4d1b2a7f8b9ab059998a6c/html5/thumbnails/3.jpg)
SEY of Arradiance Samples
0 200 400 600 8000.0
0.5
1.0
1.5
2.0
2.5
3.0
3.5
Sec
onda
ry E
lect
ron
Yie
ld (p
er P
rimar
y)
Primary Electron Energy (eV)
ARR1 1 2 3 4 5
•No clear trend between scans
•Each scan was approximately 5 minutes long
•Approximately 200nA (electrons) continuous
![Page 4: Characterization of Arradiance Samples and B33 Float Glass Slade J. Jokela](https://reader036.vdocuments.us/reader036/viewer/2022082510/5a4d1b2a7f8b9ab059998a6c/html5/thumbnails/4.jpg)
SEY of Arradiance Samples
0 200 400 600 800 1000
0.5
1.0
1.5
2.0
2.5
3.0
3.5
Sec
onda
ry E
lect
ron
Yie
ld (p
er p
rimar
y)
Primary Electron Energy (eV)
ARR1 Raw ARR1 FFT-Filtered
•FFT Filtered (Low pass of 0.05 eV-1)
![Page 5: Characterization of Arradiance Samples and B33 Float Glass Slade J. Jokela](https://reader036.vdocuments.us/reader036/viewer/2022082510/5a4d1b2a7f8b9ab059998a6c/html5/thumbnails/5.jpg)
SEY of Arradiance Samples
0 200 400 600 8000.0
0.5
1.0
1.5
2.0
2.5
3.0
3.5
Sec
onda
ry E
lect
ron
Yie
ld (p
er p
rimar
y)
Primary Electron Energy (eV)
ARR1 Deviation ARR2 Deviation ARR3 Deviation
•Average of 5 sequential scans
•Each of the 5 spectra were FFT-filtered
•Standard Deviation is shown
•It would appear that each of these samples produces similar SEY
![Page 6: Characterization of Arradiance Samples and B33 Float Glass Slade J. Jokela](https://reader036.vdocuments.us/reader036/viewer/2022082510/5a4d1b2a7f8b9ab059998a6c/html5/thumbnails/6.jpg)
b33 side 2 - 600ev to 0ev.1
O KL L O 1s O 2s O 2pO 2p3/ 2O 2p1/ 2
C KLL C 1s
C 2p3/2C 2p1/2C 2p
Ca LMM Ca 2s Ca 2p1/2Ca 2p3/2Ca 2p
Ca 3s
Ca 3p3/2
Ca 3p
Ca 3p1/2
Sn 3s Sn MNNSn 3p1/2
Sn 3pSn 3p3/2
Sn 3d3/2Sn 3d5/2Sn 3d
Sn 4s Sn 4p1/2Sn 4p3/2Sn 4p
Sn 4d5/2Sn 4d3/2
Sn 4d
Sn 5pSn 5s
Sn 5p1/2Sn 5p3/2
Si LMMSi 2s
Si 2p1/2Si 2pSi 2p3/2
Si 3sSi 3pSi 3p3/2Si 3p1/2
Si KLLSb 3sSb 3p1/2
Sb MNN Sb 3p
Sb 3p3/2Sb 3d3/2
Sb 3d5/2Sb 3d
Sb 4s
Sb 4pSb 4p3/2Sb 4p1/2
Sb 4d3/2Sb 4d5/2Sb 4d
Sb 5sSb 5pSb 5p3/2Sb 5p1/2
As 3s
As 3p1/2As 3pAs 3p3/2
As 3d
As 3d3/2As 3d5/2
As LMMAs 4p3/2As 4pAs 4p1/2
x 104
2
4
6
8
10
CPS
500 400 300 200 100 0Bi nding E nergy (eV)
O
SnCa C
Si*, Sb, As
O*CaAsSbSn
•B33 was tested in early January
•*Most likely candidate for visible peak(s)
•Data is shifted by about 7eV due to insulating-nature of glass
•Peak shift is not constant across entire spectrum due to insulating-nature of glass as well as chemical shifts
•Sb and As will not be resolvable for this sample due to interference with both O and Si
•B270 was not tested as a possible solution was found that determined which side of the glass was the float side
B33 Float Glass
![Page 7: Characterization of Arradiance Samples and B33 Float Glass Slade J. Jokela](https://reader036.vdocuments.us/reader036/viewer/2022082510/5a4d1b2a7f8b9ab059998a6c/html5/thumbnails/7.jpg)
This Week
• Will continue testing Al2O3 samples from our ALD group
• MatSci Division ISM-Day on Friday• Troubleshooting and hopefully fixing the
UV-light source– He plasma forms between anode and HV-
input rather than between anode and cathode.